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On Complexity of Jackiw-Teitelboim Gravity

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arxiv 1811.09028 v2 pith:S62GB2W6 submitted 2018-11-22 hep-th

Mohsen Alishahiha This is my paper · ORCID
classification hep-th
keywords complexitygravityjackiw-teitelboimbehinddimensionalhorizonactionassuming
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Using "complexity=action" proposal we compute complexity for Jackiw-Teitelboim gravity assuming that a UV cutoff enforces us to have a cut off behind the horizon. We find that the resultant complexity exhibits the late time linear growth. It is also consistent with the case where the corresponding Jackiw-Teitelboim gravity is obtained by dimensional reduction from higher dimensional gravities. To this work certain counter term on the cut off surface behind horizon is needed.

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Cited by 4 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Toward Krylov-based holography in double-scaled SYK

    hep-th 2025-10 unverdicted novelty 6.0 of 10

    Establishes a threefold duality linking Krylov complexity growth rate to wormhole velocity and proper momentum in DSSYK holography, with higher moments capturing replica wormholes and Krylov entropy equaling parent-ge...

  2. Wedge Holographic Complexity in Karch-Randall Braneworld

    hep-th 2024-12 conditional novelty 6.0 of 10

    For a wedge black string with fluctuating branes, the Complexity=Action growth rate gains a constant edge-mode term while Complexity=Volume gains a fluctuation-squared correction, breaking the naive equivalence of the...

  3. Jackiw-Teitelboim Model Coupled to Conformal Matter in the Semi-Classical Limit

    hep-th 2019-08 conditional novelty 6.0 of 10

    For JT gravity with conformal matter, the generalized entropy defined from the horizon dilaton plus matter entanglement is monotonic along the event horizon and along future Q-screens under the null energy condition, ...

  4. An Infalling Observer and Behind the Horizon Cutoff

    hep-th 2019-08 conditional novelty 4.0 of 10

    For an eternal black hole, the interior partition function factorizes as the square of the exterior one, fixing the behind-the-horizon cutoff in terms of the UV cutoff.

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